{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,11]],"date-time":"2025-10-11T02:17:01Z","timestamp":1760149021581,"version":"build-2065373602"},"reference-count":28,"publisher":"MDPI AG","issue":"13","license":[{"start":{"date-parts":[[2023,6,28]],"date-time":"2023-06-28T00:00:00Z","timestamp":1687910400000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"funder":[{"name":"Shanghai Rising-Star Program","award":["23QA1411000","22ZR1472400","23ZR1473200","2022YFF0504100","CXJJ-22S019"],"award-info":[{"award-number":["23QA1411000","22ZR1472400","23ZR1473200","2022YFF0504100","CXJJ-22S019"]}]},{"name":"Natural Science Foundation of Shanghai","award":["23QA1411000","22ZR1472400","23ZR1473200","2022YFF0504100","CXJJ-22S019"],"award-info":[{"award-number":["23QA1411000","22ZR1472400","23ZR1473200","2022YFF0504100","CXJJ-22S019"]}]},{"name":"National Key R&amp;D Program of China","award":["23QA1411000","22ZR1472400","23ZR1473200","2022YFF0504100","CXJJ-22S019"],"award-info":[{"award-number":["23QA1411000","22ZR1472400","23ZR1473200","2022YFF0504100","CXJJ-22S019"]}]},{"name":"Key Laboratory of Space Active Opto-electronics Technology, CAS","award":["23QA1411000","22ZR1472400","23ZR1473200","2022YFF0504100","CXJJ-22S019"],"award-info":[{"award-number":["23QA1411000","22ZR1472400","23ZR1473200","2022YFF0504100","CXJJ-22S019"]}]}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Remote Sensing"],"abstract":"<jats:p>As part of China\u2019s Tianwen-1 Mars mission, the Mars Surface Composition Detector (MarSCoDe) instrument on the Zhurong rover adopts laser-induced breakdown spectroscopy (LIBS) to perform chemical component detection of the materials on the Martian surface. However, it has always been a challenging issue to achieve high accuracy in LIBS quantification. This study investigated the effect of chemometrics and spectral data preprocessing approaches on LIBS quantification accuracy based on different chemometrics algorithms and diverse preprocessing methods. A total of 2340 LIBS spectra were collected from 39 kinds of geochemical samples by a laboratory duplicate model of the MarSCoDe instrument. The samples and the MarSCoDe laboratory model were placed in a simulated Martian atmosphere environment based on equipment called the Mars-Simulated Detection Environment Experiment Platform (MarSDEEP). To quantify the concentration of MgO in the samples, we employed two common LIBS chemometrics; i.e., partial least squares (PLS) and a back-propagation neural network (BPNN). Meanwhile, in addition to necessary routine preprocessing such as dark subtraction, we used five specific preprocessing approaches, namely intensity normalization, baseline removal, Mg-peak wavelength correction, Mg-peak feature engineering, and concentration range reduction. The results indicated that the performance of the BPNN was better than that of the PLS and that the preprocessing of Mg-peak wavelength correction had the most prominent effect to improve the quantification accuracy. The results of this study are expected to provide inspiration for the processing and analysis of the in situ LIBS data acquired by MarSCoDe on Mars.<\/jats:p>","DOI":"10.3390\/rs15133311","type":"journal-article","created":{"date-parts":[[2023,6,29]],"date-time":"2023-06-29T01:15:47Z","timestamp":1688001347000},"page":"3311","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":0,"title":["Investigation into the Affect of Chemometrics and Spectral Data Preprocessing Approaches upon Laser-Induced Breakdown Spectroscopy Quantification Accuracy Based on MarSCoDe Laboratory Model and MarSDEEP Equipment"],"prefix":"10.3390","volume":"15","author":[{"ORCID":"https:\/\/orcid.org\/0009-0008-3839-6940","authenticated-orcid":false,"given":"Ziyi","family":"Liu","sequence":"first","affiliation":[{"name":"School of Physics and Optoelectronic Engineering, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China"},{"name":"University of Chinese Academy of Sciences, Beijing 100049, China"}]},{"given":"Luning","family":"Li","sequence":"additional","affiliation":[{"name":"Key Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China"}]},{"given":"Weiming","family":"Xu","sequence":"additional","affiliation":[{"name":"School of Physics and Optoelectronic Engineering, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China"},{"name":"Key Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China"}]},{"given":"Xuesen","family":"Xu","sequence":"additional","affiliation":[{"name":"School of Physics and Optoelectronic Engineering, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-9807-9583","authenticated-orcid":false,"given":"Zhicheng","family":"Cui","sequence":"additional","affiliation":[{"name":"School of Physics and Optoelectronic Engineering, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China"},{"name":"University of Chinese Academy of Sciences, Beijing 100049, China"}]},{"given":"Liangchen","family":"Jia","sequence":"additional","affiliation":[{"name":"School of Physics and Optoelectronic Engineering, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China"},{"name":"University of Chinese Academy of Sciences, Beijing 100049, China"}]},{"given":"Wenhao","family":"Lv","sequence":"additional","affiliation":[{"name":"School of Physics and Optoelectronic Engineering, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China"},{"name":"University of Chinese Academy of Sciences, Beijing 100049, China"}]},{"given":"Zhihui","family":"Shen","sequence":"additional","affiliation":[{"name":"School of Physics and Optoelectronic Engineering, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China"},{"name":"University of Chinese Academy of Sciences, Beijing 100049, China"}]},{"given":"Rong","family":"Shu","sequence":"additional","affiliation":[{"name":"School of Physics and Optoelectronic Engineering, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China"},{"name":"Key Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China"}]}],"member":"1968","published-online":{"date-parts":[[2023,6,28]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"114657","DOI":"10.1016\/j.icarus.2021.114657","article-title":"Geological Characteristics of China\u2019s Tianwen-1 Landing Site at Utopia Planitia, Mars","volume":"370","author":"Wu","year":"2021","journal-title":"Icarus"},{"key":"ref_2","doi-asserted-by":"crossref","first-page":"64","DOI":"10.1007\/s11214-021-00836-5","article-title":"The MarSCoDe Instrument Suite on the Mars Rover of China\u2019s Tianwen-1 Mission","volume":"217","author":"Xu","year":"2021","journal-title":"Space Sci. 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